BEGIN:VCALENDAR
VERSION:2.0
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BEGIN:VEVENT
SUMMARY:Machine Vision Applications
DTSTART;VALUE=DATE-TIME:20210528T051000Z
DTEND;VALUE=DATE-TIME:20210528T053000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4111@events01.synchrotron.org.au
DESCRIPTION:Speakers: Matthew Rees (ANSTO)\nAt the Centre for Accelerator 
 Science (CAS) in ANSTO Lucas Heights\, we have recently been evaluating so
 lutions incorporating the use of Machine Vision as a tool for improving ou
 r systems and operations.\nThis talk will provide a brief introduction to 
 Machine Vision and its applications in general industry.  We will discuss 
 how Machine Vision has been used previously here at CAS and explore its fu
 ture potential.\n\nhttps://events01.synchrotron.org.au/event/136/contribut
 ions/4111/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4111/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Physics Instrumentation Engineers of Australia - Let's Collaborate
  More!
DTSTART;VALUE=DATE-TIME:20210528T040000Z
DTEND;VALUE=DATE-TIME:20210528T042000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4104@events01.synchrotron.org.au
DESCRIPTION:Speakers: David Brodrick (ANU)\nHaving been engaged in the dev
 elopment of radio telescopes\, neutron facilities\, and optical and infrar
 ed astronomy facilities\, I can't help observe that many of the engineerin
 g building blocks are precisely the same. At the same time I see that\, in
  practice\, so few of the instrumentation engineers in Australia have the 
 opportunity to share experiences with\, or learn lessons from counterparts
  at other Australian physics facilities.\n\nThe ANU Research School of Ast
 ronomy and Astrophysics have recently allocated strategic funding to suppo
 rt better collaboration and communication with our instrumentation counter
 parts supporting other realms of science in Australia.\n\nThe intent of th
 is talk is to provide a background to the initiative while leaving time fo
 r discussion on ways in which better engagement may enrich us all.\n\nhttp
 s://events01.synchrotron.org.au/event/136/contributions/4104/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4104/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Script based GUI builder for instrument control and data treatment
DTSTART;VALUE=DATE-TIME:20210527T235000Z
DTEND;VALUE=DATE-TIME:20210528T001000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4107@events01.synchrotron.org.au
DESCRIPTION:Speakers: Norman Xiong (ANSTO)\nA new feature has been added t
 o the Gumtree software that allows users to create their own graphical use
 r interfaces for controlling the neutron scattering instruments and treati
 ng data. Users without any GUI design experience can write simple Python s
 cripts in this software environment\, and the system will automatically ge
 nerate the GUI accordingly. These scripts can be used for a mixed of purpo
 ses such as driving devices\, collecting neutrons\, treating the data\, an
 d plotting them.\n\nhttps://events01.synchrotron.org.au/event/136/contribu
 tions/4107/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4107/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Science NET
DTSTART;VALUE=DATE-TIME:20210528T053000Z
DTEND;VALUE=DATE-TIME:20210528T055000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4116@events01.synchrotron.org.au
DESCRIPTION:https://events01.synchrotron.org.au/event/136/contributions/41
 16/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4116/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Open Discussion
DTSTART;VALUE=DATE-TIME:20210528T061000Z
DTEND;VALUE=DATE-TIME:20210528T063000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4115@events01.synchrotron.org.au
DESCRIPTION:General open discussion\n\nhttps://events01.synchrotron.org.au
 /event/136/contributions/4115/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4115/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Architecture and maintenance of accelerator control system
DTSTART;VALUE=DATE-TIME:20210528T055000Z
DTEND;VALUE=DATE-TIME:20210528T061000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4108@events01.synchrotron.org.au
DESCRIPTION:Speakers: Nikolai Lobanov (ANU)\, Peter Linardakis (Australian
  National University)\, Daniel Tempra (ANU)\, Stephen Battison (ANU)\nUnde
 r current University re-structure\, we have limited resources allocated fo
 r upgrades and regular maintenance of the HIAF control system. We will str
 ucture this talk as an open discussion session dedicated to the current st
 atus and future development of HIAF control system and potentially engagin
 g some collaborators from the delegation to form an advisory/workforce gro
 up to address those issues.\n\nhttps://events01.synchrotron.org.au/event/1
 36/contributions/4108/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4108/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Docker for Beamline Controls
DTSTART;VALUE=DATE-TIME:20210528T042000Z
DTEND;VALUE=DATE-TIME:20210528T044000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4114@events01.synchrotron.org.au
DESCRIPTION:Speakers: Stephen Mudie (ANSTO)\nThe SAXS/WAXS beamline at the
  Australian Synchrotron has been successfully using docker containers to r
 un epics IOCs\, including Galil motor controllers and GigE video cameras\,
  since 2016. This system has proved extremely reliable\, easy to maintain\
 , and self documenting. The current system uses Docker Swarm for High Avai
 lability/Redundancy\, and where possible reuses docker images for multiple
  IOCs\, with configuration injected at run time. This talk will give an in
 troduction to Docker and present an overview of the implementation of Dock
 er on the Australian Synchrotron SAXS/WAXS beamline.\n\nhttps://events01.s
 ynchrotron.org.au/event/136/contributions/4114/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4114/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Automatically generated engineering GUIs
DTSTART;VALUE=DATE-TIME:20210528T034000Z
DTEND;VALUE=DATE-TIME:20210528T040000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4095@events01.synchrotron.org.au
DESCRIPTION:Speakers: Andraz Pozar (Australian Synchrotron)\nAt the Austra
 lian Synchrotron we will use a combination of tools to capture the operati
 onal area controls system structure and from it generate engineering GUIs 
 for that area at a click of a button.\n\nhttps://events01.synchrotron.org.
 au/event/136/contributions/4095/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4095/
END:VEVENT
BEGIN:VEVENT
SUMMARY:CSBS - Control System Breakdown Structure
DTSTART;VALUE=DATE-TIME:20210528T032000Z
DTEND;VALUE=DATE-TIME:20210528T034000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4113@events01.synchrotron.org.au
DESCRIPTION:Speakers: Rosemary Waghorn (Australian Synchrotron)\nAt the Au
 stralian Synchrotron we use a tool to allow entry of the operational area 
 controls system structure which includes both the assembly and control hie
 rarchies. This tool also includes auto generate of component (devices\, co
 ntrollers\, hosts\, IOCs) names\, and API endpoints that can be used by ot
 her applications.\n\nhttps://events01.synchrotron.org.au/event/136/contrib
 utions/4113/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4113/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Float64 Motor Record
DTSTART;VALUE=DATE-TIME:20210528T020000Z
DTEND;VALUE=DATE-TIME:20210528T022000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4112@events01.synchrotron.org.au
DESCRIPTION:Speakers: Nader Afshar (Australian Synchrotron - ANSTO)\nIn th
 e Australian Synchrotron\, we have standardised our motion controls based 
 on Omron's PowerBrickLV(r)\, an advanced and versatile controller platform
 .\n\nIn order to utilise the advanced features of these controllers while 
 maintaining the complexity that comes with the versatile and multi-purpose
 d controller\, DLS developers team led the community by setting up a softw
 are stack with modules in the controller firmware up to the motor record.\
 n\nIn the Controls Systems team\, we took on the task of advancing the DLS
  software stack and Motor Record to meet our new requirements for PPMAC na
 mely: supporting fractional readbacks in engineering units from controller
 \, improved performance of the driver\, additional protection functions at
  the controller level and streamlined routines e.g. homing routines\, with
 out backward compatibility requirements. \n\nNow we are testing our beta v
 ersion of the software stack\, with an improved Motor Record\, driver and 
 IOC templates.\n\nhttps://events01.synchrotron.org.au/event/136/contributi
 ons/4112/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4112/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Interfacing to Xilinx Alveo Accelerator Cards using caproto and py
 OpenCL
DTSTART;VALUE=DATE-TIME:20210528T014000Z
DTEND;VALUE=DATE-TIME:20210528T020000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4110@events01.synchrotron.org.au
DESCRIPTION:Speakers: Euan Troup (CSIRO Astronomy and Space)\nXilinx Alveo
  FPGA processing cards are used for DSP in beamformers for both CSIRO Park
 es telescope CryoPAF and SKA-Low Telescope Correlator and Beamformer proje
 cts. The telescope control systems use EPICS and TANGO respectively. We ha
 ve used pyOpenCL to create a control-system-independent layer to the beamf
 ormer firmware in the Alveo card then used caproto to create a Python IOC 
 for interface to the Parkes control system. This talk will describe these 
 systems with details of the caproto Python script\n\nhttps://events01.sync
 hrotron.org.au/event/136/contributions/4110/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4110/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Developing a High Voltage Generator controller for the 2MV Tandetr
 on accelerator
DTSTART;VALUE=DATE-TIME:20210528T012000Z
DTEND;VALUE=DATE-TIME:20210528T014000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4106@events01.synchrotron.org.au
DESCRIPTION:Speakers: Nikolas Paneras ()\, Yasser Yasser Mafi Nejad ()\nTh
 e aim of this project is to develop a controller to run the High Voltage G
 enerator (HVG) for the 2MV Tandetron accelerator (Small Tandem Accelerator
  for Research (STAR)) at ANSTO.\n\nThe HVG is a solid state voltage multip
 lier used instead of a belt or pellet chain to generate the high potential
  for the accelerator terminal.\n\nThe current HVG controller PCB is damage
 d and is running in a static\, fixed frequency mode. The current controlle
 r is constructed of obsolete components that have no direct replacements. 
 The repair of this PCB in not a feasible option.\n\nThe new control hardwa
 re is based on a NI cRIO-9035 PLC using a NI9401 (Ultra-fast digital outpu
 t)\, NI9403 (Digital Input/Output) and a NI9205 (Analogue Input). We are u
 sing LabVIEW 2019 for the software development environment.\n\nThis PLC co
 nsists of a FPGA and a Real Time unit within an ARM based processor. The a
 ccelerator controller is in charge of tracking the resonant frequency of t
 he accelerator. This is achieved within the FPGA section by implementing a
  phase-locked loop (PLL). The output stage IGBTs are controlled also by th
 e FPGA using PWM in real parallel execution. Moreover\, the interlock syst
 em will be developed in Real Time controller.\n\nThe implemented wideband 
 PLL will maximise power delivery efficiency to the HVG. The PLL free-runni
 ng VCO is able to tune from 35 kHz to 47 kHz (25%) with a lock in range of
  40.7 to 41.3 kHz. This enables the controller to precisely track the drif
 t in the resonant frequency of the HVG.  \n\nThe controller can also preci
 sely vary the width of the pulse (PWM) from 1% to 99% (operational range f
 rom 5 – 30 %) with the resolution of 1% at the entire frequency band. Th
 is will enable the accelerator to run at different voltages terminals. \n\
 nExperimental results shows that our new HVG control system not only runs 
 the accelerator efficiently and safely\, but also provides remote monitori
 ng and upgradability.\n\nhttps://events01.synchrotron.org.au/event/136/con
 tributions/4106/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4106/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Fast ORM Measurement for Australian Synchrotron
DTSTART;VALUE=DATE-TIME:20210528T010000Z
DTEND;VALUE=DATE-TIME:20210528T012000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4102@events01.synchrotron.org.au
DESCRIPTION:Speakers: Simin Chen (ANSTO)\nThe fast ORM measurement system 
 would be capable of reducing the measurement time of the storage ring’s 
 corrector to position response matrix from 15 minutes down to around 1 min
 ute.\n\nThe fast ORM measurement system is designed to generate sinusoidal
  excitation of the electron beam with or without FOFB correction data for 
 fast response measurements. It is also equipped with a white noise generat
 or for closed loop gain analysis. With a much larger FPGA\, the FOFB corre
 ction data can be encoded as UDP packets and sent to IOCs for archiving an
 d offline analysis.\n\nhttps://events01.synchrotron.org.au/event/136/contr
 ibutions/4102/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4102/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Computer Control Operation and Future Upgrade Plan in STAR Acceler
 ator Facility at ANSTO
DTSTART;VALUE=DATE-TIME:20210528T001000Z
DTEND;VALUE=DATE-TIME:20210528T003000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4105@events01.synchrotron.org.au
DESCRIPTION:Speakers: JIAN WANG (CAS ANSTO)\nSTAR is a 2MV tandetron accel
 erator that can perform both IBA and AMS analyses. It has three ion source
 s which include two duoplasmatron sources for hydrogen and helium\, and a 
 solid target sputter source used primarily for ionising carbon samples for
  AMS. The STAR accelerator currently has 3 beamlines\, a multi-elemental s
 urface analysis beamline (SIBA1)\, a high-resolution depth profiling and i
 rradiation beamline (SIBA2)\, and a 14C beamline (AMS).\nThis presentation
  will firstly introduce the current computer control system\, and look at 
 its history and developments. These include partial modification of the or
 iginal C14-OS package in Windows NT\, and upgrade from Windows NT to Windo
 ws XP. \nDue to the age of the system\, and the base hardware\, operation 
 and maintenance of the control system has become problematic. Consideratio
 n for a future upgrade of the STAR computer control system are in there ea
 rly stage. This presentation will also explore two possible upgrading and 
 replacement options.\n\nhttps://events01.synchrotron.org.au/event/136/cont
 ributions/4105/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4105/
END:VEVENT
BEGIN:VEVENT
SUMMARY:MEX Crystal Spectrometer
DTSTART;VALUE=DATE-TIME:20210527T233000Z
DTEND;VALUE=DATE-TIME:20210527T235000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4109@events01.synchrotron.org.au
DESCRIPTION:Speakers: Danny Wong ()\nThe Crystal Spectrometer is one of th
 e first equipment arrived onsite for ANSTO's BR-IGHT program.\n- Where it 
 came from?\n- What changes were made?\n- How it is currently implemented?\
 n- Engineering GUI\n- video of Spectrometer in Action\n- What's next?\n\nh
 ttps://events01.synchrotron.org.au/event/136/contributions/4109/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4109/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Advanced Instrumentation Technology Centre at ANU
DTSTART;VALUE=DATE-TIME:20210527T231000Z
DTEND;VALUE=DATE-TIME:20210527T233000Z
DTSTAMP;VALUE=DATE-TIME:20260814T122421Z
UID:indico-contribution-136-4103@events01.synchrotron.org.au
DESCRIPTION:Speakers: David Brodrick (ANU)\nThe Advanced Instrumentation T
 echnology Centre (AITC)\, at ANU's Mount Stromlo Observatory\, is a largel
 y self-funding body\, receiving contracts to develop optical and infrared 
 instrumentation for some of the world's largest telescopes. We also host t
 he Australian Space Test Facility and are a node of the Australian Astrono
 mical Optics (AAO) consortium\, operating and providing instrumentation fo
 r Australia's premier telescopes.\n\nThis presentation provides a brief in
 troduction to the AITC\, some of our current projects and the control syst
 ems used to realise them.\n\nhttps://events01.synchrotron.org.au/event/136
 /contributions/4103/
LOCATION:Zoom
URL:https://events01.synchrotron.org.au/event/136/contributions/4103/
END:VEVENT
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